Instrumental
Mean-combined stacks in counts, with FITS header metadata for photometric conversion.
All DR1 images are astrometrically calibrated. The current release provides instrumental, calibrated, and star-removed mean stacks for 2116 fields, together with downloadable bundles of individual exposures for each field.
Mean-combined stacks in counts, with FITS header metadata for photometric conversion.
Fields converted to Janskies using the field-specific photometric zero point.
Calibrated mean fields with star-removal processing applied.
Per-field bundles of the component exposures used to form the mean stack.
Instrumental images include the MAGZP header keyword, which is used to convert
measured counts to calibrated AB magnitudes.
mag(MDW) = -2.5 * log10(measured flux [counts]) + MAGZP
The magnitude zero point is determined by comparing MDW instrumental Hα magnitudes to catalog-matched IGAPS AB Hα magnitudes and aligning the stellar locus with the synthetic early-A reddening line.
For calibrated and star-removed products, the FITS unit is converted to Janskies.
mag(MDW) = -2.5 * log10(measured flux [Jy] / 3631 [Jy])
The filter below narrows the displayed fields by RA and Dec. Individual field bundles are linked through the per-field CGI download route.